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Ultralight bosonic dark matter called fuzzy dark matter (FDM) has attracted much attention as an alternative to the cold dark matter. An intriguing feature of the FDM model is the presence of a soliton core, a stable dense core formed at…

宇宙学与河外天体物理 · 物理学 2022-12-07 Atsushi Taruya , Shohei Saga

Soliton cores at the center of fuzzy dark matter (FDM) halos provide a promising way to distinguish FDM from other dark matter models. However, the relation between solitons and their host halos remains contentious. Here, we rigorously…

宇宙学与河外天体物理 · 物理学 2025-07-18 Pin-Yu Liao , Guan-Ming Su , Hsi-Yu Schive , Alexander Kunkel , Hsinhao Huang , Tzihong Chiueh

In the fuzzy dark matter (FDM) model, gravitationally collapsed objects always consist of a solitonic core located within a virialised halo. Although various numerical simulations have confirmed that the collapsed structure can be described…

宇宙学与河外天体物理 · 物理学 2022-04-27 Hei Yin Jowett Chan , Elisa G. M. Ferreira , Simon May , Kohei Hayashi , Masashi Chiba

We examine the nonlinear structure of gravitationally collapsed objects that form in our simulations of wavelike cold dark matter ($\psi$DM), described by the Schr\"{o}dinger-Poisson (SP) equation with a particle mass $\sim 10^{-22} {\rm…

We investigate phenomenologically the viability of fuzzy dark matter (FDM). We do this by confronting the predictions of the model, in particular, the formation of a solitonic core at the center of dark matter halos, with a homogeneous and…

星系天体物理 · 物理学 2024-03-15 Andrés Bañares-Hernández , Andrés Castillo , Jorge Martin Camalich , Giuliano Iorio

We present the results of a full cosmological simulation with the new code SCALAR, where dark matter is in form of fuzzy dark matter, described by a light scalar field with a mass of $m_{\rm B} = 2.5 \times 10^{-22}$ eV and evolving…

宇宙学与河外天体物理 · 物理学 2022-06-08 Mattia Mina , David F. Mota , Hans A. Winther

Fuzzy Dark Matter (FDM) comprised of ultralight ($m \sim 10^{-22}~\rm{eV}$) boson particles has received significant attention as a viable alternative to Cold Dark Matter (CDM), as it approximates CDM on large scales ($\gtrsim 1$ Mpc) while…

宇宙学与河外天体物理 · 物理学 2024-02-28 Connor A. Painter , Michael Boylan-Kolchin , Philip Mocz , Mark Vogelsberger

We explore the effect of a supermassive black hole (SMBH) on the density profile of a fuzzy dark matter (FDM) soliton core at the centre of a dark matter halo. We numerically solve the Schr\"odinger-Poisson equations, treating the black…

星系天体物理 · 物理学 2020-03-11 Elliot Yarnell Davies , Philip Mocz

We present zoom-in simulations of fuzzy dark matter (FDM) halos including baryons and star-formation with sufficient resolution to follow the formation and evolution of central solitons. We find that their properties are determined by the…

宇宙学与河外天体物理 · 物理学 2020-04-16 Jan Veltmaat , Bodo Schwabe , Jens C. Niemeyer

A Fuzzy Dark Matter (FDM) halo consists of a soliton core close to the center and an NFW-like density profile in the outer region. Previous investigations found that the soliton core exhibits temporal oscillations and random walk excursions…

宇宙学与河外天体物理 · 物理学 2021-01-13 Xinyu Li , Lam Hui , Tomer D. Yavetz

We examine the impact of moderate repulsive self-interactions on fuzzy dark matter halos generated by merging smaller Gaussian density concentrations. We study the size of the core and the granules, the spatial dependence of the field's…

宇宙学与河外天体物理 · 物理学 2025-12-31 Milos Indjin , Nick Keepfer , I-Kang Liu , Nick P. Proukakis , Gerasimos Rigopoulos

Wave (fuzzy) dark matter ($\psi$DM) consists of ultralight bosons, featuring a solitonic core within a granular halo. Here we extend $\psi$DM to two components, with distinct particle masses $m$ and coupled only through gravity, and…

宇宙学与河外天体物理 · 物理学 2023-04-18 Hsinhao Huang , Hsi-Yu Schive , Tzihong Chiueh

(abridged)Scalar field dark matter (SFDM) made of bosons has become a popular alternative to the CDM paradigm, especially for its potential to cure the so-called "small-scale problems" of CDM. Cosmological simulations have determined that…

宇宙学与河外天体物理 · 物理学 2025-06-19 Matthias Stallovits , Tanja Rindler-Daller

Fuzzy Dark Matter (FDM), consisting of ultralight bosons ($m_{\rm b} \sim 10^{-22}\ \rm eV$), is an intriguing alternative to Cold Dark Matter. Numerical simulations that solve the Schr\"odinger-Poisson (SP) equation show that FDM halos…

In this work we study the possibility of modeling the dark matter content in galaxies as a core-halo model consisting of self-gravitating, self-interacting fermions. For the core of the halo, the dark matter fermions are degenerate, while…

高能物理 - 唯象学 · 物理学 2025-12-03 Fabian Hernandez-Gutierrez , Juan Barranco

We study the impact of self-interactions on the structure and evolution of scalar field dark matter (SFDM) halos. Using three-dimensional Gross-Pitaevskii-Poisson simulations of multiple soliton mergers, we explore both repulsive and…

宇宙学与河外天体物理 · 物理学 2026-05-13 Jessica N. López-Sánchez , Erick Munive-Villa , Tanja Rindler-Daller

Fuzzy dark matter (FDM) is an intriguing candidate alternative to the standard cold dark matter (CDM). The FDM model predicts that dark halos have characteristic core structures generated by the effect of quantum pressure, which is…

宇宙学与河外天体物理 · 物理学 2024-07-17 Hiroki Kawai , Ayuki Kamada , Kohei Kamada , Naoki Yoshida

Fuzzy dark matter (FDM) made of ultra-light bosonic particles is a viable alternative to cold dark matter (CDM) with clearly distinguishable small-scale features in collapsed structures. On large scales, it behaves gravitationally like CDM…

宇宙学与河外天体物理 · 物理学 2022-05-11 Bodo Schwabe , Jens C. Niemeyer

The fuzzy dark matter model (FDM, also known as quantum wave dark matter model) argues that light bosons with a mass of $\sim10^{-22}{\;{\rm eV}}$ are a possible candidate for dark matter in the Universe. One of the most important…

星系天体物理 · 物理学 2020-02-12 Zhi Li , Juntai Shen , Hsi-Yu Schive

Fuzzy dark matter (FDM) is composed of ultra-light bosons having a de Broglie wavelength that is comparable to the size of the stellar component of galaxies at typical galactic velocities. FDM behaves like cold dark matter on large scales.…

星系天体物理 · 物理学 2021-07-07 Ben Bar-Or , Jean-Baptiste Fouvry , Scott Tremaine
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